<?xml version="1.0" encoding="UTF-8"?><!DOCTYPE article  PUBLIC "-//NLM//DTD Journal Publishing DTD v3.0 20080202//EN" "http://dtd.nlm.nih.gov/publishing/3.0/journalpublishing3.dtd"><article xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink" dtd-version="3.0" xml:lang="en" article-type="research article"><front><journal-meta><journal-id journal-id-type="publisher-id">JAMP</journal-id><journal-title-group><journal-title>Journal of Applied Mathematics and Physics</journal-title></journal-title-group><issn pub-type="epub">2327-4352</issn><publisher><publisher-name>Scientific Research Publishing</publisher-name></publisher></journal-meta><article-meta><article-id pub-id-type="doi">10.4236/jamp.2015.34051</article-id><article-id pub-id-type="publisher-id">JAMP-55818</article-id><article-categories><subj-group subj-group-type="heading"><subject>Articles</subject></subj-group><subj-group subj-group-type="Discipline-v2"><subject>Physics&amp;Mathematics</subject></subj-group></article-categories><title-group><article-title>
 
 
  Modelling Textural Anisotropy of Magnetic Susceptibility of Banded Iron Formations
 
</article-title></title-group><contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>William</surname><given-names>W. Guo</given-names></name><xref ref-type="aff" rid="aff1"><sub>1</sub></xref><xref ref-type="corresp" rid="cor1"><sup>*</sup></xref></contrib></contrib-group><aff id="aff1"><label>1</label><addr-line>School of Engineering &amp;amp; Technology, Central Queensland University, North Rockhampton, Australia</addr-line></aff><author-notes><corresp id="cor1">* E-mail:<email>w.guo@cqu.edu.au</email></corresp></author-notes><pub-date pub-type="epub"><day>20</day><month>04</month><year>2015</year></pub-date><volume>03</volume><issue>04</issue><fpage>405</fpage><lpage>410</lpage><history><date date-type="received"><day>January</day>	<month>2015</month>	</date></history><permissions><copyright-statement>&#169; Copyright  2014 by authors and Scientific Research Publishing Inc. </copyright-statement><copyright-year>2014</copyright-year><license><license-p>This work is licensed under the Creative Commons Attribution International License (CC BY). http://creativecommons.org/licenses/by/4.0/</license-p></license></permissions><abstract><p>
 
 
   Anisotropy of magnetic susceptibility (AMS) of banded iron formations (BIFs) is characterized by high anisotropy and well-developed bedding-parallel magnetic foliation. Since most previous studies were focused on palaeomagneism of BIFs and BIF-derived iron ores, little effort has been made to further understand this special type of AMS for BIFs. A detailed theoretical analysis, incorporating with the previous experimental data, is made to understand the formative mechanism of this special anisotropy for BIFs. The good consistence between the theoretical and experimental results demonstrates that this type of anisotropy is likely caused by the layered structure of BIFs, and thus verifies the term of textural anisotropy for BIFs. Theoretical analysis also shows that in the negligence of the inter-layer magnetic action BIF’s apparent anisotropy increases with an increase in intrinsic susceptibility of magnetic layers, but decreases with an increase in length-to- diameter ratio of the magnetic layer. 
 
</p></abstract><kwd-group><kwd>Textural Anisotropy of Magnetic Susceptibility (AMS)</kwd><kwd> Banded Iron Formation (BIF)</kwd><kwd> Theoretical and Experimental Modelling</kwd><kwd> Hamersley Province</kwd></kwd-group></article-meta></front><body><sec id="s1"><title>1. Introduction</title><p>Banded iron formation, usually abbreviated to BIF, is the lithological term for a chemical sediment consisting of a “thinly layered or laminated rock in which chert (or its metamorphic equivalent) alternates with layers that are composed mainly of iron minerals; the iron content typically is in the range 20% - 35% and the SiO<sub>2</sub> is in the range 40% - 50%” [<xref ref-type="bibr" rid="scirp.55818-ref1">1</xref>]. High-grade iron ores derived from BIFs form the main reserves of cheaply exploitable iron in Africa, Australia, India, South America, and Russia. Magnetite BIFs in the United States, Canada and China are also mined due to the easy concentration of magnetite by magnetic separation.</p><p>Anisotropy of magnetic susceptibility (AMS) of single crystal grains is caused by either magnetocrystalline anisotropy or shape anisotropy [<xref ref-type="bibr" rid="scirp.55818-ref2">2</xref>] [<xref ref-type="bibr" rid="scirp.55818-ref3">3</xref>]. The magnitude of AMS of natural rocks depends on both the anisotropy of individual magnetic particles and the degree of their alignment. The preferred orientation of crystallographic axes commonly controls grain shape and determines the AMS for the vast majority of minerals [<xref ref-type="bibr" rid="scirp.55818-ref4">4</xref>]. The AMS of most natural rocks is formed if there is a net statistical alignment of crystallographic axes, which could be acquired in the original diagenesis, or later metamorphism, deformation and other physical and chemical events. In BIFs, however, ferromagnetic grains are concentrated along some bands. In such a case the magnetic interactions among the ferromagnetic grains can generate an overall magnetic behavior completely different from the behavior of both individual grains and the statistical alignment of crystallographic axes of these grains.</p><p>AMS of BIFs is often characterized by high anisotropy [<xref ref-type="bibr" rid="scirp.55818-ref5">5</xref>]-[<xref ref-type="bibr" rid="scirp.55818-ref8">8</xref>] and well-developed bedding-parallel magnetic foliation [<xref ref-type="bibr" rid="scirp.55818-ref7">7</xref>]-[<xref ref-type="bibr" rid="scirp.55818-ref9">9</xref>]. This type of anisotropy was called the textural anisotropy [<xref ref-type="bibr" rid="scirp.55818-ref10">10</xref>]. Since most of previous studies were focused on palaeomagneism of BIFs and BIF-derived iron ores, little effort has been made to further understand this special type of AMS for BIFs. In this paper, some AMS results of Hamersley BIFs are presented. A detailed theoretical analysis is made to understand the mechanism of the formation of this special anisotropy for BIFs. The theoretical model is then tested by the experimental data using artificial BIF samples given in [<xref ref-type="bibr" rid="scirp.55818-ref5">5</xref>].</p></sec><sec id="s2"><title>2. AMS of BIFs in the Hamersley Province</title><p>The Hamersley Province in the northwest of Western Australia hosts extensive BIFs and high-grade hematite/martite ores. Fresh BIFs in the Hamersley Province commonly contain ~30 wt% magnetite [<xref ref-type="bibr" rid="scirp.55818-ref11">11</xref>] [<xref ref-type="bibr" rid="scirp.55818-ref12">12</xref>], but they are normally covered by an overlying weathered BIF layer that is tens to ~100 m thick [<xref ref-type="bibr" rid="scirp.55818-ref12">12</xref>]. In weathered BIFs, magnetite content varies from &lt;0.5 wt% to &lt;15 wt% and consequently the bulk susceptibility of weathered BIFs is much lower than that of fresh BIFs. Typical structure of BIFs in the Hamersley Province is shown in <xref ref-type="fig" rid="fig1">Figure 1</xref>.</p><p>The features of AMS of four selected BIF sites are shown in <xref ref-type="fig" rid="fig2">Figure 2</xref>. For each site, the average position of the minimum susceptibility axes is very close to the pole position of bedding, normally with a difference less than 10˚. The average degree of anisotropy of these BIF sites varies from 1.16 to 1.69, and the lineation is almost equal to 1.0. This means that the susceptibility along the bedding is almost isotropic. Thus, all these sites show a well-developed magnetic foliation parallel or sub-parallel to bedding, called textural anisotropy [<xref ref-type="bibr" rid="scirp.55818-ref10">10</xref>].</p></sec><sec id="s3"><title>3. Theoretical Analysis of the Formation of Textural Anisotropy for BIFs</title><p>For a standard cylindrical BIF sample (<xref ref-type="fig" rid="fig3">Figure 3</xref>), assuming it consists of alternating strong magnetic (intrinsic susceptibility<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/55818x3.png" xlink:type="simple"/></inline-formula>) and non-magnetic layers (N layers in total). The thickness of each layer, however, can differ. If a magnetic field is applied parallel to the layers, the apparent (or measured) susceptibility of the whole sample parallel to the layer <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/55818x4.png" xlink:type="simple"/></inline-formula> is given as [<xref ref-type="bibr" rid="scirp.55818-ref5">5</xref>]:</p><disp-formula id="scirp.55818-formula112"><label>, (1)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/55818x5.png"  xlink:type="simple"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/55818x6.png" xlink:type="simple"/></inline-formula> is the volume fraction of magnetic layer material; <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/55818x7.png" xlink:type="simple"/></inline-formula>is the demagnetization factor of the sample as a whole in the direction of parallel to the layer.</p><p>If a magnetic field is applied normal to the layers, the apparent susceptibility of the whole sample normal to the layer <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/55818x8.png" xlink:type="simple"/></inline-formula> is given as:</p><disp-formula id="scirp.55818-formula113"><label>, (2)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/55818x9.png"  xlink:type="simple"/></disp-formula><fig id="fig1"  position="float"><label><xref ref-type="fig" rid="fig1">Figure 1</xref></label><caption><title> Summary of stratification scales within BIFs of the Hamersley Province. White re- presents chert-rich unit and other patterns represent iron-rich unit. Black is for magnetite (modified from [<xref ref-type="bibr" rid="scirp.55818-ref12">12</xref>])</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/55818x10.png"/></fig><fig id="fig2"  position="float"><label><xref ref-type="fig" rid="fig2">Figure 2</xref></label><caption><title> AMS of BIFs from Hamersley Province of Western Australia</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/55818x11.png"/></fig><fig id="fig3"  position="float"><label><xref ref-type="fig" rid="fig3">Figure 3</xref></label><caption><title> Schematic section of a cylindrical BIF sample</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/55818x12.png"/></fig><p>where <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/55818x13.png" xlink:type="simple"/></inline-formula> and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/55818x14.png" xlink:type="simple"/></inline-formula> are the apparent susceptibility and demagnetization factor of the ith magnetic layer in the direction of normal to the layer.</p><p>From Equations (1) and (2), the apparent anisotropy <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/55818x15.png" xlink:type="simple"/></inline-formula> of the sample can be expressed as</p><disp-formula id="scirp.55818-formula114"><label>. (3)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/55818x16.png"  xlink:type="simple"/></disp-formula><p>In case of the equal thickness of each magnetic layer, this apparent anisotropy becomes</p><disp-formula id="scirp.55818-formula115"><label>, (4)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/55818x17.png"  xlink:type="simple"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/55818x18.png" xlink:type="simple"/></inline-formula> <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/55818x19.png" xlink:type="simple"/></inline-formula> is the demagnetization factor of a single magnetic layer normal to the layer. If there is no magnetic interaction between the adjacent magnetic layers, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/55818x19.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/55818x20.png" xlink:type="simple"/></inline-formula>is determined independently by the geometry of a single magnetic layer. For a standard samples,<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/55818x19.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/55818x20.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/55818x21.png" xlink:type="simple"/></inline-formula>. Thus Equation (4) is further simplified as</p><disp-formula id="scirp.55818-formula116"><label>. (5)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/55818x22.png"  xlink:type="simple"/></disp-formula><p>For a thin cylindrical magnetic layer, its demagnetization factor along the cylindrical axis is known as [<xref ref-type="bibr" rid="scirp.55818-ref5">5</xref>]:</p><disp-formula id="scirp.55818-formula117"><label>(6)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/55818x23.png"  xlink:type="simple"/></disp-formula><p>where p is the length-to-diameter ratio of the cylindrical magnetic layer.</p><p>From Equations (5) and (6), theoretical apparent anisotropy of a BIF sample can be determined in the negligence of the inter-layer magnetic action. <xref ref-type="fig" rid="fig4">Figure 4</xref> shows some of these theoretical results, with<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/55818x24.png" xlink:type="simple"/></inline-formula>. It is clear that the apparent anisotropy increases with an increase in intrinsic susceptibility of the magnetic layers (<xref ref-type="fig" rid="fig4">Figure 4</xref>(a)), but decreases with an increase in length-to-diameter ratio of the magnetic layer (<xref ref-type="fig" rid="fig4">Figure 4</xref>(b)).</p><p>With further increase in the intrinsic susceptibility of the magnetic layers, the apparent anisotropy should differ from these theoretical results. This is because magnetic interactions between the magnetic layers get stronger with increasing intrinsic susceptibility. In such a condition, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/55818x25.png" xlink:type="simple"/></inline-formula>in Equation (5) becomes an empirical constant [<xref ref-type="bibr" rid="scirp.55818-ref5">5</xref>], which may be better determined by using contemporary computational methods like neural networks [<xref ref-type="bibr" rid="scirp.55818-ref13">13</xref>] [<xref ref-type="bibr" rid="scirp.55818-ref14">14</xref>] or the combination with statistical means [<xref ref-type="bibr" rid="scirp.55818-ref15">15</xref>], rather than statistics alone.</p></sec><sec id="s4"><title>4. Discussion and Conclusion</title><p>Jahren [<xref ref-type="bibr" rid="scirp.55818-ref5">5</xref>] gave some experimental results for artificial BIF samples. Some of the results are listed in <xref ref-type="table" rid="table1">Table 1</xref>. <xref ref-type="fig" rid="fig5">Figure 5</xref> shows the theoretical results of apparent anisotropy using Equations (5) and (6), with a<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/55818x26.png" xlink:type="simple"/></inline-formula>. The corresponding experimental results from <xref ref-type="table" rid="table1">Table 1</xref> are plotted and numbered in all the cases.</p><p><xref ref-type="fig" rid="fig5">Figure 5</xref>(a) shows that the two measured points <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/55818x27.png" xlink:type="simple"/></inline-formula> distribute close to the theoretical curve. This good coincidence continues up to ~1.6 SI. This means that in the case of <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/55818x27.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/55818x28.png" xlink:type="simple"/></inline-formula> and the adjacent magnetic layers separating by the same ratio, the magnetic interaction between magnetic layers is insignificant when <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/55818x27.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/55818x28.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/55818x29.png" xlink:type="simple"/></inline-formula> SI. <xref ref-type="fig" rid="fig5">Figure 5</xref>(b) shows that the three measured points <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/55818x27.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/55818x28.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/55818x29.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/55818x30.png" xlink:type="simple"/></inline-formula> are close to the theoretical curve, but</p><fig id="fig4"  position="float"><label><xref ref-type="fig" rid="fig4">Figure 4</xref></label><caption><title> Theoretical curves of apparent anisotropy (A<sub>a</sub>) versus: (a) intrinsic susceptibility (κ), and (b) length-to-diameter ratio of the magnetic layer (p). The volume fraction of magnetic layer material (v<sub>m</sub>) is 1/3</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/55818x31.png"/></fig><fig id="fig5"  position="float"><label><xref ref-type="fig" rid="fig5">Figure 5</xref></label><caption><title> Theoretical curves of apparent anisotropy (A<sub>a</sub>) versus intrinsic susceptibility (κ) with length-to-diameter ratio of the magnetic layer (p) of 0.1250 (a) and 0.0625 (b). Black dots are corresponding experimental results of measured anisotropy using artificial samples in [<xref ref-type="bibr" rid="scirp.55818-ref5">5</xref>]. The volume fraction of magnetic layer material (v<sub>m</sub>) is &#189;</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/55818x32.png"/></fig><table-wrap id="table1" ><label><xref ref-type="table" rid="table1">Table 1</xref></label><caption><title> Experimental results of apparent anisotropy of artificial layered samples [<xref ref-type="bibr" rid="scirp.55818-ref5">5</xref>]</title></caption><table><tbody><thead><tr><th align="center" valign="middle" >Point number</th><th align="center" valign="middle" >Thickness of magnetic layer (cm)</th><th align="center" valign="middle" >Intrinsic susceptibility (SI)</th><th align="center" valign="middle" >Apparent anisotropy</th><th align="center" valign="middle" >Number of magnetic layers</th><th align="center" valign="middle" >Ratio of magnetic to non-magnetic layer thicknesses</th></tr></thead><tr><td align="center" valign="middle" >1</td><td align="center" valign="middle" >0.27</td><td align="center" valign="middle" >0.2261</td><td align="center" valign="middle" >1.17</td><td align="center" valign="middle" >4</td><td align="center" valign="middle" >1</td></tr><tr><td align="center" valign="middle" >2</td><td align="center" valign="middle" >0.27</td><td align="center" valign="middle" >1.6328</td><td align="center" valign="middle" >1.71</td><td align="center" valign="middle" >4</td><td align="center" valign="middle" >1</td></tr><tr><td align="center" valign="middle" >3</td><td align="center" valign="middle" >0.14</td><td align="center" valign="middle" >0.2261</td><td align="center" valign="middle" >1.16</td><td align="center" valign="middle" >8</td><td align="center" valign="middle" >1</td></tr><tr><td align="center" valign="middle" >4</td><td align="center" valign="middle" >0.14</td><td align="center" valign="middle" >0.6531</td><td align="center" valign="middle" >1.39</td><td align="center" valign="middle" >8</td><td align="center" valign="middle" >1</td></tr><tr><td align="center" valign="middle" >5</td><td align="center" valign="middle" >0.14</td><td align="center" valign="middle" >1.6328</td><td align="center" valign="middle" >1.75</td><td align="center" valign="middle" >8</td><td align="center" valign="middle" >1</td></tr></tbody></table></table-wrap><p>this good coincidence can only continue up to &lt;1.5 SI. Point 5 with <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/55818x33.png" xlink:type="simple"/></inline-formula> SI deviates obviously from the theoretical curve. This is because when the magnetic layers are thinner and closer to each other (p gets smaller), magnetic interactions between the magnetic layers get stronger with increasing intrinsic susceptibility.</p><p>Since the real BIF samples are more complicated than the artificial BIF samples, no direct comparison can be made between the theoretical results and the results of the real BIF samples from this study and other previous studies. However, the good correspondence between the theoretical and the measured results from the artificial BIF samples has demonstrated that the banded texture of BIFs is likely to count for the special type of AMS carried by BIFs, i.e., high anisotropy with a well-developed magnetic foliation parallel or sub-parallel to bedding. Thus this study verifies the term of textural anisotropy for BIFs given in [<xref ref-type="bibr" rid="scirp.55818-ref10">10</xref>].</p></sec><sec id="s5"><title>Cite this paper</title><p>William W. Guo, (2015) Modelling Textural Anisotropy of Magnetic Susceptibility of Banded Iron Formations. Journal of Applied Mathematics and Physics,03,405-410. doi: 10.4236/jamp.2015.34051</p></sec></body><back><ref-list><title>References</title><ref id="scirp.55818-ref1"><label>1</label><mixed-citation publication-type="other" xlink:type="simple">James, H.L. (1983) Distribution of Banded Iron-Formation in Space and Time. In: Iron-Formation: Facts and Problems, Elsevier, Amsterdam, 471-490. http://dx.doi.org/10.1016/S0166-2635(08)70053-7</mixed-citation></ref><ref id="scirp.55818-ref2"><label>2</label><mixed-citation publication-type="other" xlink:type="simple">Tarling, D.H. and Hrouda, F. (1993) The Magnetic Anisotropy of Rocks. Chapman &amp; Hall, London.</mixed-citation></ref><ref id="scirp.55818-ref3"><label>3</label><mixed-citation publication-type="other" xlink:type="simple">Dunlop, D.J. and Ozdemir, O. (1997) Rock Magnetism. Cambridge University Press, Cambridge. 
http://dx.doi.org/10.1017/CBO9780511612794</mixed-citation></ref><ref id="scirp.55818-ref4"><label>4</label><mixed-citation publication-type="other" xlink:type="simple">Rochette, P., Jackson, M. and Aubourg, C. (1992) Rock Magnetism and the Interpretation of Anisotropy of Magnetic Susceptibility. Reviews of Geophysics, 30, 209-226. http://dx.doi.org/10.1029/92RG00733</mixed-citation></ref><ref id="scirp.55818-ref5"><label>5</label><mixed-citation publication-type="other" xlink:type="simple">Jahren, C.E. (1963) Magnetic Susceptibility of Bedded Iron Formation. Geophysics, 28, 756-766. 
http://dx.doi.org/10.1190/1.1439268</mixed-citation></ref><ref id="scirp.55818-ref6"><label>6</label><mixed-citation publication-type="other" xlink:type="simple">Clark, D.A. and Schmidt, P. (1986) Magnetic Properties of the Banded-Iron Formations of the Hamersley Group, WA. CSIRO Division of Mineral Physics, AMIRA Report 1638.</mixed-citation></ref><ref id="scirp.55818-ref7"><label>7</label><mixed-citation publication-type="other" xlink:type="simple">Schmidt, P. and Clark, D.A. (1994) Palaeomagnetism and Magnetic Anisotropy of Proterozoic Banded-Iron Formations and Iron Ores of the Hamersley Basin, Western Australia. Precambian Research, 69, 133-155. 
http://dx.doi.org/10.1016/0301-9268(94)90083-3</mixed-citation></ref><ref id="scirp.55818-ref8"><label>8</label><mixed-citation publication-type="other" xlink:type="simple">Guo, W. (1999) Magnetic Petrophysics and Density Investigations of the Hamersley Province, Western Australia: Implications for Magnetic and Gravity Interpretation. The University of Western Australia, Perth.</mixed-citation></ref><ref id="scirp.55818-ref9"><label>9</label><mixed-citation publication-type="other" xlink:type="simple">Guo, W.W. (In Press) Mathematical Model of Anisotropy of Magnetic Susceptibility (AMS). Journal of Applied Mathematics and Physics.</mixed-citation></ref><ref id="scirp.55818-ref10"><label>10</label><mixed-citation publication-type="other" xlink:type="simple">Porath, H. and Chamalaun, F.H. (1968) Palaeomagnetism of Australian Haematite Ore Bodies, II, Western Australia. Geophysical Journal Royal Astronomical Society, 15, 253-264. http://dx.doi.org/10.1111/j.1365-246X.1968.tb00184.x</mixed-citation></ref><ref id="scirp.55818-ref11"><label>11</label><mixed-citation publication-type="other" xlink:type="simple">Trendall, A.F. (1983) Introduction, in Iron-Formation: Facts and Problems. Elsevier, Amsterdam, 1-12. 
http://dx.doi.org/10.1016/S0166-2635(08)70040-9</mixed-citation></ref><ref id="scirp.55818-ref12"><label>12</label><mixed-citation publication-type="other" xlink:type="simple">Morris, R.C. (1993) Genetic Modelling for Banded Iron-Formation of the Hamersley Group, Pilbara Craton, Western Australia. Precambrian Research, 60, 243-286. http://dx.doi.org/10.1016/0301-9268(93)90051-3</mixed-citation></ref><ref id="scirp.55818-ref13"><label>13</label><mixed-citation publication-type="other" xlink:type="simple">Guo, W.W. (2010) A Novel Application of Neural Networks for Instant Iron-Ore Grade Estimation. Expert Systems with Applications, 37, 8729-8735. http://dx.doi.org/10.1016/j.eswa.2010.06.043</mixed-citation></ref><ref id="scirp.55818-ref14"><label>14</label><mixed-citation publication-type="other" xlink:type="simple">Li, M.M., Guo, W., Verma, B., Tickle, K. and O’Connor, J. (2009) Intelligent Methods for Solving Inverse Problems of Backscattering Spectra with Noise: A Comparison between Neural Networks and Simulated Annealing. Neural Computing and Applications, 18, 423-430. http://dx.doi.org/10.1007/s00521-008-0219-x</mixed-citation></ref><ref id="scirp.55818-ref15"><label>15</label><mixed-citation publication-type="other" xlink:type="simple">Guo, W.W., Li, M.M., Whymark, G. and Li, Z.X. (2009) Mutual Complement between Statistical and Neural Network Approaches for Rock Magnetism Data Analysis. Expert Systems with Applications, 36, 9678-9682. 
http://dx.doi.org/10.1016/j.eswa.2008.11.045</mixed-citation></ref></ref-list></back></article>